SDO HMI 2011-11-25 14:58:57 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 90.53 | 367.30 | 67.36 | 269.37 | 19.52 | 192.09 | -44.98 | 64.68 | 0.7378 | -111.2 | -142.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.65 | 209.74 | 1.86 | 146.55 | 19.10 | 194.65 | -42.42 | 64.26 | 0.7101 | -714.6 | -391.0 | |
| 6.59 | -1.00 | 4.61 | -1.00 | 18.82 | 194.70 | -42.38 | 64.62 | 0.7085 | -927.7 | 999999 | |
| 26.10 | -1.00 | 18.26 | -1.00 | 18.32 | 194.51 | -42.56 | 65.37 | 0.7088 | -1025.1 | 999999 | |
| 2.40 | -1.00 | 1.67 | -1.00 | 17.70 | 194.66 | -42.42 | 66.15 | 0.7050 | -664.0 | 999999 | |
| 2.48 | 5.73 | 1.77 | 4.10 | 19.11 | 193.49 | -43.59 | 64.70 | 0.7229 | -622.4 | -451.2 | |
| 10.18 | 25.76 | 7.29 | 18.48 | 18.73 | 193.27 | -43.81 | 65.29 | 0.7241 | -724.3 | -352.7 | |
| 0.00 | 0.34 | 0.00 | 0.25 | 19.16 | 192.82 | -44.26 | 64.89 | 0.7304 | -333.0 | -463.2 | |
| 1.63 | -6.00 | 1.17 | -6.00 | 18.66 | 192.81 | -44.27 | 65.55 | 0.7288 | -415.7 | 999999 | |
| 0.51 | 2.74 | 0.37 | 1.99 | 19.43 | 192.55 | -44.53 | 64.63 | 0.7343 | -557.5 | -457.9 | |
| 2.40 | 6.08 | 1.76 | 4.46 | 19.83 | 192.09 | -44.98 | 64.28 | 0.7404 | -452.8 | 137.5 | |
| 0.00 | 1.11 | 0.00 | 0.81 | 19.06 | 192.37 | -44.71 | 65.19 | 0.7349 | -455.0 | -382.4 | |
| 0.00 | 5.65 | 0.00 | 4.13 | 19.18 | 192.19 | -44.88 | 65.09 | 0.7372 | -203.0 | -99.2 | |
| 0.60 | 4.11 | 0.44 | 3.04 | 20.14 | 191.71 | -45.36 | 64.02 | 0.7455 | -468.4 | -340.7 | |
| 0.00 | 0.77 | 0.00 | 0.57 | 19.48 | 191.64 | -45.44 | 64.90 | 0.7441 | 408.0 | 364.1 | |
| 1.71 | 7.27 | 1.28 | 5.42 | 20.32 | 191.28 | -45.79 | 63.95 | 0.7506 | -408.5 | 87.3 | |
| 0.00 | 1.03 | 0.00 | 0.76 | 19.79 | 191.35 | -45.73 | 64.61 | 0.7482 | 340.0 | 319.2 | |
| 1.11 | 5.31 | 0.83 | 3.98 | 19.53 | 190.90 | -46.18 | 65.10 | 0.7520 | 792.5 | 629.4 | |
| 1.88 | -17.00 | 1.42 | -17.00 | 19.62 | 190.59 | -46.48 | 65.09 | 0.7555 | 590.0 | 999999 | |
| 0.00 | 0.94 | 0.00 | 0.71 | 20.08 | 190.28 | -46.80 | 64.61 | 0.7602 | 640.0 | 619.8 | |
| 2.05 | 21.31 | 1.56 | 16.30 | 19.89 | 190.03 | -47.05 | 64.93 | 0.7622 | 655.5 | 529.9 | |
| 6.50 | -20.00 | 4.99 | -20.00 | 20.32 | 189.76 | -47.32 | 64.48 | 0.7662 | 780.2 | 999999 | |
| 0.00 | 0.77 | 0.00 | 0.60 | 21.63 | 189.06 | -48.01 | 63.08 | 0.7773 | 720.0 | 566.6 | |
| 0.60 | 3.00 | 0.47 | 2.36 | 21.62 | 188.78 | -48.30 | 63.18 | 0.7800 | 623.9 | 486.2 | |
| 0.00 | 0.68 | 0.00 | 0.57 | 24.60 | 187.00 | -50.07 | 60.19 | 0.8059 | 489.0 | 441.8 | |
| 2.57 | 5.39 | 2.10 | 4.41 | 21.74 | 186.86 | -50.22 | 63.65 | 0.7988 | 668.2 | 560.5 | |
| 17.46 | 50.15 | 14.57 | 41.89 | 22.33 | 186.16 | -50.91 | 63.15 | 0.8069 | 791.0 | 448.7 | |
| 0.00 | 0.94 | 0.00 | 0.77 | 21.42 | 186.51 | -50.56 | 64.15 | 0.8012 | 546.0 | 477.0 | |
| 1.11 | -26.00 | 0.94 | -26.00 | 22.77 | 185.58 | -51.50 | 62.81 | 0.8135 | 332.2 | 999999 | |
| 0.00 | 1.20 | 0.00 | 1.00 | 21.88 | 185.88 | -51.19 | 63.78 | 0.8083 | 549.0 | 488.6 | |
| 0.00 | 0.77 | 0.00 | 0.66 | 22.76 | 185.32 | -51.75 | 62.90 | 0.8158 | 239.0 | 181.2 | |
| 0.00 | 1.20 | 0.00 | 1.01 | 22.19 | 185.52 | -51.56 | 63.52 | 0.8125 | 369.0 | 335.1 | |
| 0.00 | 1.20 | 0.00 | 1.02 | 22.47 | 185.16 | -51.91 | 63.29 | 0.8164 | 280.0 | 257.5 | |
| 0.00 | 1.03 | 0.00 | 0.87 | 21.77 | 185.27 | -51.81 | 64.09 | 0.8137 | 533.0 | 410.6 | |
| 0.00 | 2.31 | 0.00 | 1.98 | 22.28 | 184.95 | -52.12 | 63.58 | 0.8178 | 462.0 | 328.9 | |
| 0.00 | 0.77 | 0.00 | 0.68 | 22.34 | 183.59 | -53.49 | 63.88 | 0.8301 | 305.0 | 246.2 | |
| Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
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that the umbra consists of fragmented regions which cannot be separated without losing umbral area. In this way several spots (intensity minima in the umbra) have a common umbra, e.g. -2 means that the given spot shares an umbra with spot No.2, and the common U value is indicated at spot No.2. |
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| Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
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that several umbras have a common penumbra, e.g. -7 means that the given umbra shares a penumbra with umbra No.7, and the WS value is indicated at No.7. |
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| Corr. U | - Corrected umbra area in millionths of solar hemisphere, for negative values see above | |
| Corr. WS | - Corrected whole spot area in millionths of solar hemisphere, for negative values see above | |
| B | - Heliographic latitude B; positive: North, negative: South | |
| L | - Heliographic longitude L | |
| LCM | - Longitudinal distance from the Sun's central meridian | |
| Pos. angle | - Position angle | |
| r | - Distance from the centre of Sun's disc in terms of Sun's radius | |
| MU | - Mean magnetic field within the umbra contour averaged the pixel values with sign. | |
| MP | - Mean magnetic field within the penumbra contour averaged the pixel values with sign. | |